On the spectrum of a gaseous nebula of pure hydrogen, II

Calculations of the optical continuum of a nebula of pure hydrogen were carried out, taking into account, together, with the recombination emission, the two-photon emission and the continuous emission in the reaction of formation of the negative ion of hydrogen. It is found that these processes beco...

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Autor principal: Gerola, H.
Otros Autores: Panagia, N.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: Kluwer Academic Publishers 1970
Acceso en línea:Registro en Scopus
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100 1 |a Gerola, H. 
245 1 3 |a On the spectrum of a gaseous nebula of pure hydrogen, II 
260 |b Kluwer Academic Publishers  |c 1970 
270 1 0 |m Gerola, H.; Departmento de Fisica, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, Argentina 
506 |2 openaire  |e Política editorial 
504 |a Allen, C.W., (1963) Astrophyscial Quantities, , The Athlone Press, London 
504 |a Baker, J.G., Menzel, D.H., Physical Processes in Gaseous Nebulae. III. The Balmer Decrement. (1938) The Astrophysical Journal, 88, p. 52 
504 |a Boardman, W.J., (1964) Astrophys. J., (90), p. 185 
504 |a Burgess, A., (1965) Memoirs Roy Astron. Soc., 69, p. 1 
504 |a Capriotti, E., Mean Escape Probabilities of Line Photons. (1965) The Astrophysical Journal, 142, p. 1101 
504 |a Caputo, F., Panagia, N., Gerola, H., (1970) Astrophys. Letters, 5, p. 275 
504 |a Carson, T.R., (1966) J. Quant. Spectr. Radiative Transfer, 6, p. 563 
504 |a Chamberlain, J.W., Collisional Excitation of Hydrogen in a Gaseous Nebula. (1953) The Astrophysical Journal, 117, p. 387 
504 |a Doughty, N.A., Fraser, P.A., McEachran, R.P., The Bound-Free Absorption Coefficient of the Negative Hydrogen Ion (1966) Monthly Notices of the Royal Astronomical Society, 132, p. 255 
504 |a Doughty, N.A., Fraser, P.A., The Free-Free Absorption Coefficient of the Negative Hydrogen Ion (1966) Monthly Notices of the Royal Astronomical Society, 132, p. 267 
504 |a Geltman, S., (1964) Astrophys. J., 141, p. 376 
504 |a Gerola, H., Panagia, N., (1968) Astrophys. Space Sci, 2, p. 285 
504 |a Glasco, H.P., Zirin, H., (1964) Astrophys. J., (90), p. 193 
504 |a Greenstein, J.L., Page, T., Negative Hydrogen Ions in Planetary Nebulae. (1951) The Astrophysical Journal, 114, p. 106 
504 |a Gulyaev, R.A., (1967) Soviet Astron., 10 (5), p. 761 
504 |a Haro, G., Hα Emission Stars and Peculiar Objects in the Orion Nebula. (1953) The Astrophysical Journal, 117, p. 73 
504 |a Kaler, J.B., (1968) Astrophys. Letters, 1, p. 227 
504 |a Karzas, W. I. and Latter, R.: 1961, Astrophys. J. Suppl. Ser.6, N. 55; Lambert, D.L., Pagel, B.E.J., The Dissociation Equilibrium of H- in Stellar Atmospheres (1968) Monthly Notices of the Royal Astronomical Society, 141, p. 299 
504 |a Maffei, P. 1963, Oss. Astrof. Univ. Padova n. 140; O'Dell, C.R., Photoelectric Spectrophotometry of MHα 328-116 (1967) The Astrophysical Journal, 149, p. 373 
504 |a Parker, R.A.R., The Spectrum of a Nebula Under Conditions of Collisional Excitation and Ionization (1964) The Astrophysical Journal, 139, p. 208 
504 |a Peimbert, M., Temperature Determinations of H II Regions (1967) The Astrophysical Journal, 150, p. 825 
504 |a Van Blerkom, D., The Effect of Diffuse Ionizing Radiation in Collisionally Excited Nebulae (1968) The Astrophysical Journal, 152, p. 963 
504 |a Van Blerkom, D., Hummer, D.G., The Ionization Structure of Planetary Nebulae--VI: The Lyman Continuum Problem (1967) Monthly Notices of the Royal Astronomical Society, 137, p. 353 
520 3 |a Calculations of the optical continuum of a nebula of pure hydrogen were carried out, taking into account, together, with the recombination emission, the two-photon emission and the continuous emission in the reaction of formation of the negative ion of hydrogen. It is found that these processes become predominant when thermal collisions are responsible for the excitation of the nebula. Mixed conditions of excitation, that is by both radiation and collisions, have also been studied. The optical continuum is found to be very sensitive to the excitation conditions, so that a very small contribution of collisional ionizations to the total number of ionizations is sufficient to sensibly modify the appearance of the continuum. © 1970 D. Reidel Publishing Company.  |l eng 
593 |a Departmento de Fisica, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, Argentina 
593 |a Laboratorio di Astrofisica, Frascati, Italy 
700 1 |a Panagia, N. 
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